Neutrino condensates at center of galaxies as background for the MSW mechanism

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dc.creatorCapozziello, S.
dc.creatorIovane, G.
dc.creatorLambiase, G.
dc.date2003-04-01
dc.date.accessioned2026-07-07T10:47:36Z
dc.date.available2026-07-07T10:47:36Z
dc.descriptionThe possibility is explored that neutrino condensates, possible candidates for the explanation of very massive objects in galactic centers, could act as background for the Mikheyev-Smirnov-Wolfeinstein mechanism responsible of neutrino oscillations. Assuming a simple neutrino star model with constant density, the lower limit of the mass squared difference of neutrino oscillations is inferred. Consequences on neutrino asymmetry are discussed.
dc.description5 pages, to appear in Mod. Phys. Lett. A
dc.identifierhttps://arxiv.org/abs/astro-ph/0304013
dc.identifierhttp://arxiv.org/abs/astro-ph/0304013
dc.identifierMod.Phys.Lett.A18:905-912,2003
dc.identifierdoi:10.1142/S0217732303009988
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183588
dc.subjectAstrophysics
dc.titleNeutrino condensates at center of galaxies as background for the MSW mechanism
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